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- W2038067243 abstract "Ways in which the radiation-driven thermal instability might affect the structure of the solar atmosphere are considered. It is found that the ultimate state of the medium is highly sensitive to the evolving modal content of the perturbation in that both the initial modal composition and the extent of mode coupling determine the final structure of the atmosphere. It is also found that the condensation process generates highly rotational flows during and after the transition to a new stable state." @default.
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- W2038067243 date "1988-01-01" @default.
- W2038067243 modified "2023-10-16" @default.
- W2038067243 title "Nonlinear thermal instability in the solar transition region" @default.
- W2038067243 doi "https://doi.org/10.1086/165920" @default.
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